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Jonathan F.C. Herman Aline K. Zimmer Johannes P.J. Reijneveld Kathryn L. Dunlop Yu Takahashi Simon Tardivel Daniel J. Scheeres 《Acta Astronautica》2014
This paper presents a mission analysis comparison of human missions to asteroids using two distinct architectures. The objective is to determine if either architecture can reduce launch mass with respect to the other, while not sacrificing other performance metrics such as mission duration. One architecture relies on chemical propulsion, the traditional workhorse of space exploration. The second combines chemical and electric propulsion into a hybrid architecture that attempts to utilize the strengths of each, namely the short flight times of chemical propulsion and the propellant efficiency of electric propulsion. The architectures are thoroughly detailed, and accessibility of the known asteroid population is determined for both. The most accessible asteroids are discussed in detail. Aspects such as mission abort scenarios and vehicle reusability are also discussed. Ultimately, it is determined that launch mass can be greatly reduced with the hybrid architecture, without a notable increase in mission duration. This demonstrates that significant performance improvements can be introduced to the next step of human space exploration with realistic electric propulsion system capabilities. This leads to immediate cost savings for human exploration and simultaneously opens a path of technology development that leads to technologies enabling access to even further destinations in the future. 相似文献
104.
E.A. Bering F.R. Chang-Díaz J.P. Squire M. Brukardt T.W. Glover R.D. Bengtson V.T. Jacobson G.E. McCaskill L. Cassady 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Plasma physics has found an increasing range of practical industrial applications, including the development of electric spacecraft propulsion systems. One of these systems, the Variable Specific Impulse Magnetoplasma Rocket (VASIMR) engine, both applies several important physical processes occurring in the magnetosphere. These processes include the mechanisms involved in the ion acceleration and heating that occur in the Birkeland currents of an auroral arc system. Auroral current region processes that are simulated in VASIMR include lower hybrid heating, parallel electric field acceleration and ion cyclotron acceleration. This paper will focus on using a physics demonstration model VASIMR to study ion cyclotron resonance heating (ICRH). The major purpose is to provide a VASIMR status report to the COSPAR community. The VASIMR uses a helicon antenna with up to 20 kW of power to generate plasma. This plasma is energized by an RF booster stage that uses left hand polarized slow mode waves launched from the high field side of the ion cyclotron resonance. The present setup for the booster uses 2–4 MHz waves with up to 20 kW of power. This process is similar to the ion cyclotron heating in tokamaks, but in the VASIMR the ions only pass through the resonance region once. The rapid absorption of ion cyclotron waves has been predicted in recent theoretical studies. These theoretical predictions have been supported with several independent measurements in this paper. The ICRH produced a substantial increase in ion velocity. Pitch angle distribution studies show that this increase takes place in the resonance region where the ion cyclotron frequency is equal to the frequency on the injected RF waves. Downstream of the resonance region the perpendicular velocity boost should be converted to axial flow velocity through the conservation of the first adiabatic invariant as the magnetic field decreases in the exhaust region of the VASIMR. In deuterium plasma, 80% efficient absorption of 20 kW of ICRH input power has been achieved. No evidence for power limiting instabilities in the exhaust beam has been observed. 相似文献
105.
Nabeel Ahmad Samia F. Gurmani Riffat M. Qureshi Talat Iqbal 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(2):927-936
The atmospheric electric Potential Gradient (PG) variation of fair-weather days at Muzaffarabad (MZF, Northern Pakistan) station is presented for the period of January 2015–October 2017. The present investigations focus on the diurnal variation of atmospheric PG on the seasonal and annual time scale. The fair-weather seasonal and annual average PG variation has revealed two peaks, i.e. a primary maximum peak and a secondary maximum peak. The average maximum PG value found is ~410?Vm?1. The results are then compared with the well-known standard oceanic Carnegie curve. The diurnal curve of PG is found to deviate from the Carnegie curve. The seasonal PG variation at MZF shows lower values during the summer (monsoon) and autumn (post-monsoon) as compared to the winter and spring (pre-monsoon) which could be due to local aerosol concentration. Global comparison of PG (%) values of the annual mean at different longitude, with MZF observatory, shows local morning and evening peaks depicting local sunrise and sunset effects on the PG. The overall outcomes will certainly contribute to further investigate the Global Electric Circuit (GEC). 相似文献
106.
战术导弹发动机无线电子干扰滤波器是确保导弹发动机战勤安全的一个重要电子产品。为了评价它的可靠性,需对其进行可靠性验证试验。据此,结合一种导弹发动机无线电干扰滤波器的可靠性验证试验,讨论了其可靠性验证试验的数学模型,试验方案设计和试验方面的有关问题。 相似文献
107.
系统采用一块单片机AT89S52作为跷跷板检测和电动车控制的核心,实现了电动车在不同状态下的往返行驶、起始和停止位置的判断,以及行驶时间的显示以及跷跷板平衡点的寻找等功能。 相似文献
108.
B. Schmieder P. DémoulinG. Aulanier 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
Solar filament eruptions play a crucial role in triggering coronal mass ejections (CMEs). More than 80% of eruptions lead to a CME. This correlation has been studied extensively during the past solar cycles and the last long solar minimum. The statistics made on events occurring during the rising phase of the new solar cycle 24 is in agreement with this finding. Both filaments and CMEs have been related to twisted magnetic fields. Therefore, nearly all the MHD CME models include a twisted flux tube, called a flux rope. Either the flux rope is present long before the eruption, or it is built up by reconnection of a sheared arcade from the beginning of the eruption. 相似文献
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110.
电火花加工放电位置检测的电测量法 总被引:1,自引:0,他引:1
介绍了应用于电火花加工放电点位置检测中的信号检测和电磁信号检测法 ,同时指出它们各自的特点。在实际应用中 ,应根据不同的加工要求来选取不同的检测方法 ,实现电火花加工的最优控制 ,从而达到最好的加工效果。 相似文献